NCERT Solutions for Class 11 Physics Chapter 6: System of Particles and Rotational Motion
Complete, topper-style NCERT Solutions for Class 11 Physics Chapter 6 System of Particles and Rotational Motion (2026-27 reprint): full revision notes on centre of mass, torque, angular momentum, equilibrium and moment of inertia, plus step-by-step answers to all 17 exercise questions (6.1–6.17) with diagrams, calculations and exam tips.
Chapter at a glance — complete revision notes
6.1 Introduction
So far we treated bodies as particles (point masses). Real bodies have finite size, so we now study extended bodies, which are systems of particles. The key idea is the centre of mass (CM). A large class of problems can be solved by treating bodies as rigid bodies: ideally, bodies with a perfectly definite and unchanging shape, so the distance between every pair of particles does not change. Real bodies are never truly rigid, but wheels, tops, steel beams, molecules and planets can often be treated as rigid.
6.1.1 What kind of motion can a rigid body have?
- Pure translation: all particles of the body have the same velocity at any instant (a block sliding down an incline without turning). Its motion is described by that of one point (the CM).
- Pure rotation about a fixed axis: every particle moves in a circle whose centre lies on the axis, e.g. a ceiling fan, a potter’s wheel, a merry-go-round; particles on the axis are at rest; all particles have the same angular velocity ω but different linear speed v = ωr.
- Combined motion: rolling (translation + rotation), e.g. a cylinder rolling down an inclined plane (Fig. 6.2: not pure translation), or a spinning top whose axis is not fixed (rotation about a point; the axis itself precesses).
6.2 Centre of mass
For a system of two particles on a line the CM is at X = (m1x1 + m2x2)/(m1 + m2): the mass-weighted average position; it lies between them, nearer to the heavier particle. In general, for n particles: R = Σmi ri/M with M = Σmi (6.4); X = Σmixi/M, Y = Σmiyi/M, Z = Σmizi/M. If the origin is the CM then Σmiri = 0.
- Continuous bodies: sums become integrals, X = (1/M)∫x dm, etc. For a body of uniform density and regular shape the CM is at the geometric centre: rod — midpoint; ring, sphere, cylinder, cube — the centre; thin disc — the centre; a triangular lamina — the centroid (intersection of medians, at 2/3 of each median from the vertex).
- The CM need not lie within the body (ring, hollow sphere, boomerang, a bent rod).
- The CM does not depend on the choice of coordinate axes: it is a property of the system.
Example 6.1. Three particles at the vertices of an equilateral triangle of side 0.5 m with masses 100 g, 150 g, 200 g (placing the 100 g mass at the origin and the 150 g mass on the x-axis): X = (150 × 0.5 + 200 × 0.25)/450 = 0.28 m, Y = (200 × 0.5 sin60°)/450 = 0.19 m. Example 6.2. Triangular lamina: it can be divided into thin strips parallel to a side, each with CM at its midpoint; so the CM lies on the median through that side; repeating for the other sides, the CM is the point where the medians meet (centroid). Example 6.3. A uniform L-shaped lamina made of three equal squares of side 1 m (mass 3 kg): each square has mass 1 kg at its centre; with the squares centred at (0.5, 0.5), (1.5, 0.5), (0.5, 1.5) m: X = Y = (0.5 + 1.5 + 0.5)/3 = 5/6 m.
6.3 Motion of centre of mass
Differentiating R = Σmiri/M: total momentum P = MV where V = dR/dt is the velocity of the CM, and M A = ΣFext (6.7–6.12): the CM of a system of particles moves as if all the mass of the system were concentrated at the CM and all the external forces were applied at that point. The internal forces cancel in pairs (third law). Consequences: the motion of the CM of a body thrown in the air is a parabola whatever the rotation or explosion of the body (Fig. 6.12); the CM of an exploding shell continues along the original parabola if the explosion is caused by internal forces only (the fragments hit the ground at positions such that their CM is at the CM’s point of landing).
6.4 Linear momentum of a system of particles
The total momentum of a system is P = Σpi = MV (6.15) and dP/dt = Fext (6.17): the rate of change of the total momentum equals the external force. Conservation of linear momentum: if Fext = 0 then P = constant, i.e. the CM moves with constant velocity (or stays at rest). Example: a heavy nucleus (radium) at rest decays into a lighter nucleus (radon) and an α particle; the two move in opposite directions with momenta of equal magnitude, so the CM stays at rest (Fig. 6.13). A child running on a trolley (Ex 6.3) cannot change the velocity of the CM of the system child + trolley.
6.5 Vector product of two vectors
The vector (cross) product a × b = (ab sinθ) n̂ is a vector of magnitude ab sinθ (θ = angle between a and b, 0 ≤ θ ≤ π) and direction perpendicular to the plane of a and b given by the right-hand screw rule (or right-hand rule). Properties: (i) a × b = −b × a (not commutative); (ii) a × (b + c) = a × b + a × c (distributive); (iii) a × a = 0, and a × b = 0 if a ∥ b; (iv) î × î = 0, î × ĵ = k̂, ĵ × k̂ = î, k̂ × î = ĵ; (v) in components a × b = (aybz − azby)î + (azbx − axbz)ĵ + (axby − aybx)k̂ (a determinant); (vi) |a × b| = area of the parallelogram formed by a and b; a · (b × c) = volume of the parallelepiped on a, b, c.
Example 6.4. For a = (3î − 4ĵ + 5k̂) and b = (−2î + ĵ − 3k̂): scalar product a·b = −6 − 4 − 15 = −25; vector product a × b = 7î − ĵ − 5k̂; |a| = √50, |b| = √14, so cosθ = −25/√700 = −0.945, θ ≈ 161°.
6.6 Angular velocity and its relation with linear velocity
For a particle in circular motion the angular velocity ω = dθ/dt (rad s−1); its direction is along the axis, given by the right-hand rule (ω is an axial vector). The linear velocity of a particle at position r from a point on the axis is v = ω × r (6.28); its magnitude is v = ωr_⊥ (r_⊥ = perpendicular distance from the axis). For rotation about a fixed axis the direction of ω is fixed, so ω is effectively a scalar and the angular acceleration α = dω/dt (6.30), a = α × r + ω × v.
6.7 Torque and angular momentum
Torque (moment of force) of a force F about a point O: τ = r × F, magnitude rF sinθ = (r sinθ)F = (force) × (perpendicular distance of the line of action); SI unit N m; direction perpendicular to the plane of r and F (right-hand rule). Angular momentum of a particle about O: l = r × p, magnitude rp sinθ; SI unit kg m2 s−1 (J s). Relation: dl/dt = r × F = τ (6.32–6.33): the time rate of change of angular momentum equals the torque (the rotational analogue of F = dp/dt). For a system of particles dL/dt = τext (internal torques cancel if the internal forces are central; the sum of internal torques is zero).
Conservation of angular momentum: if the total external torque is zero, L = constant (the rotational counterpart of the conservation of linear momentum): a particle under a central force (planets: Kepler’s law of areas), an ice skater drawing her arms in, and a diver. Example 6.5. Torque about the origin of F = (7î + 3ĵ − 5k̂) N acting at r = (î − ĵ + k̂) m: τ = r × F = (2î + 12ĵ + 10k̂) N m. Example 6.6. For a particle moving with constant velocity v, F = 0, so τ = 0 and l = r × mv is constant: l = m (r × v) and r_⊥ = constant (the perpendicular distance from the point to the line of motion).
6.8 Equilibrium of a rigid body
A rigid body is in mechanical equilibrium if (1) the total external force is zero, ΣFi = 0 (translational equilibrium: the linear momentum is constant) and (2) the total external torque is zero, Στi = Σri × Fi = 0 (rotational equilibrium: the angular momentum is constant). If the body is at rest it is in static equilibrium. Each is a vector equation, equivalent to three scalar equations; in a plane: ΣFx = 0, ΣFy = 0 and Στz = 0.
- Couple: a pair of equal and opposite forces with different lines of action. It produces rotation without translation (net force zero); its moment (torque) is F × d, where d is the perpendicular distance between the forces, and is the same about every point (Example 6.7). Examples: turning a key, a tap, a steering wheel, a compass needle in a magnetic field.
- Principle of moments (lever): for rotational equilibrium of a lever about the fulcrum F1d1 = F2d2: load arm × load = effort arm × effort; mechanical advantage MA = F2/F1 = d1/d2. Examples: a see-saw, balance, crowbar.
- Centre of gravity (CG): the point where the total gravitational torque on the body is zero, i.e. where the whole weight may be taken to act; for a body small compared with the Earth (uniform g) the CG coincides with the CM. A body is balanced when supported at its CG; it can be located by suspending the body from two points and finding the intersection of the vertical lines.
Example 6.8. A metal bar AB of length 70 cm and mass 4 kg rests on two knife edges placed 10 cm from each end, with a 6 kg load suspended 30 cm from end A. Taking moments about K1 (10 cm from A): R2 × 50 = 4g × 25 + 6g × 20 gives R2 = 4.4 kg wt = 43 N, and R1 = 10g − R2 = 5.6 kg wt = 55 N. Example 6.9. A 3 m ladder of mass 20 kg leans on a smooth wall with its foot 1 m from the wall: the wall reaction F and floor reaction N, f: N = W = 196 N; taking torques about the foot, F × 2√2 = W × 0.5, so F = W/(4√2) = 34.6 N; friction f = F = 34.6 N; the total reaction of the floor R = √(1962 + 34.62) = 199 N, at tan−1(196/34.6) ≈ 80° to the horizontal.
6.9 Moment of inertia
The kinetic energy of a rigid body rotating about a fixed axis with angular velocity ω is K = Σ½mivi2 = ½(Σmiri2)ω2 = ½ I ω2 (6.34–6.35), where I = Σmiri2 is the moment of inertia (MI) about the axis. I is the rotational analogue of mass: it measures the resistance to change in the rotational motion. It depends on the mass, on its distribution about the axis and on the choice of axis; SI unit kg m2; dimensions [M L2]. For a ring of mass M and radius R rotating about its axis: I = MR2; for two masses m1, m2 on a light rod: I = m1r12 + m2r22. The radius of gyration k is defined by I = Mk2.
| No. | Body | Axis | I |
|---|---|---|---|
| (1) | Thin circular ring, radius R | Perpendicular to plane, at centre | MR2 |
| (2) | Thin circular ring, radius R | Diameter | MR2/2 |
| (3) | Thin rod, length L | Perpendicular to rod, at mid-point | ML2/12 |
| (4) | Circular disc, radius R | Perpendicular to disc at centre | MR2/2 |
| (5) | Circular disc, radius R | Diameter | MR2/4 |
| (6) | Hollow cylinder, radius R | Axis of cylinder | MR2 |
| (7) | Solid cylinder, radius R | Axis of cylinder | MR2/2 |
| (8) | Solid sphere, radius R | Diameter | 2MR2/5 |
Table 6.1 of the NCERT text (PDF page 25). Supplementary (not in the reprint text but needed in problem solving): parallel axes theorem I = Icm + Ma2; perpendicular axes theorem (for plane laminas) Iz = Ix + Iy; for a hollow sphere I = 2MR2/3.
6.10 Kinematics of rotational motion about a fixed axis
Rotation about a fixed axis is described by the angular displacement θ, angular velocity ω = dθ/dt and angular acceleration α = dω/dt. For constant α: ω = ω0 + αt (6.36), θ = θ0 + ω0t + ½αt2 (6.37), ω2 = ω02 + 2α(θ − θ0) (6.38): the exact analogues of v = u + at, s = ut + ½at2 and v2 = u2 + 2as. Relation with linear quantities for a particle at distance r: v = ωr, at = αr, ac = ω2r.
Example 6.11. A motor wheel’s speed rises from 1200 rpm to 3120 rpm in 16 s: ω0 = 1200 × 2π/60 = 125.7 rad s−1, ω = 3120 × 2π/60 = 326.7 rad s−1; α = (326.7 − 125.7)/16 = 12.57 rad s−2; angle turned θ = ω0t + ½αt2 = 125.7 × 16 + ½(12.57)(16)2 = 3620 rad = 3620/2π = 576 revolutions.
6.11 Dynamics of rotational motion about a fixed axis
The rotational analogue of Newton’s second law: τ = I α (6.40), i.e. the net torque about the axis equals moment of inertia times angular acceleration. Work done by a torque: dW = τ dθ (6.41); power P = τ ω (6.42). The work–energy theorem for rotation: W = ½Iωf2 − ½Iωi2. The two kinds of motion run parallel (Table 6.2):
| Linear motion | Rotational motion about a fixed axis |
|---|---|
| Displacement x | Angular displacement θ |
| Velocity v = dx/dt | Angular velocity ω = dθ/dt |
| Acceleration a = dv/dt | Angular acceleration α = dω/dt |
| Mass M | Moment of inertia I |
| Force F = Ma | Torque τ = Iα |
| Work dW = F ds | Work dW = τ dθ |
| Kinetic energy K = Mv2/2 | Kinetic energy K = Iω2/2 |
| Power P = Fv | Power P = τω |
| Linear momentum p = Mv | Angular momentum L = Iω |
Example 6.12. A cord of negligible mass is wound on the rim of a flywheel of mass 20 kg and radius 20 cm; a steady pull of 25 N is applied. (a) τ = FR = 25 × 0.20 = 5.0 N m; I = ½MR2 = ½ × 20 × 0.04 = 0.4 kg m2; α = τ/I = 12.5 rad s−2. (b) Work done by the pull in unwinding 2 m: W = 25 × 2 = 50 J. (c) Angle turned = 2/0.2 = 10 rad; ω2 = 2αθ = 250; K = ½Iω2 = ½ × 0.4 × 250 = 50 J. (d) The work done equals the kinetic energy (the wheel starts from rest and there is no friction).
6.12 Angular momentum in case of rotation about a fixed axis
For a rigid body rotating about a fixed axis which is an axis of symmetry, the angular momentum along the axis is L = Iω (6.43) (in general L and ω need not be parallel), and the torque equation becomes τ = dL/dt = I dω/dt = Iα. Conservation of angular momentum (τext = 0): Iω = constant, so if I changes, ω changes inversely: I1ω1 = I2ω2.
- A skater or dancer spins faster when she pulls her arms in (I decreases, ω increases); her kinetic energy rises because she does work pulling the arms in.
- A diver curls up into a ball to spin rapidly for somersaults and stretches before entering the water.
- A person on a rotating turntable holding weights: pulling them in speeds the turntable up.
- Planets move faster near the Sun: the angular momentum about the Sun is conserved (Kepler’s second law).
- Cat uses conservation of angular momentum to land on its feet (twisting body parts in opposite senses).
Relation: K = L2/(2I): at constant L the kinetic energy increases as I decreases (the extra energy comes from the work done by the muscles of the skater: Ex 6.12).
Points to ponder and summary (NCERT)
- To describe the motion of a system of particles we use the centre of mass: M A = Fext; the internal forces do not affect it.
- The CM of a body (or system) need not lie within it.
- Torque τ = r × F and angular momentum l = r × p are vectors; dL/dt = τext.
- A rigid body is in equilibrium if ΣF = 0 and Στ = 0.
- For rotation about a fixed axis Iα = τ; L = Iω holds only for an axis of symmetry (the relation between L and ω in general is a matrix relation).
- Torque and angular momentum depend on the choice of the origin: always state it.
Ex 6.1 — Give the location of the centre of mass of a (i) sphere, (ii) cylinder, (iii) ring, and (iv) cube, each of uniform mass density. Does the centre of mass of a body necessarily lie inside the body?
Concept. The centre of mass of a body is the mass-weighted average position of its particles, R = (1/M)Σmiri. For a body of uniform mass density with a centre of symmetry, every particle at r has a partner at −r (measured from the centre of symmetry), so the sum Σmiri vanishes about that centre: the CM is at the geometric centre.
| Body (uniform density) | Location of the CM | Is it on the material of the body? |
|---|---|---|
| (i) Sphere (solid) | At the centre of the sphere | Yes (inside) |
| (ii) Cylinder | At the mid-point of the axis (the centre of the cylinder) | Yes (inside, for a solid cylinder) |
| (iii) Ring | At the centre of the ring (on the axis through the centre, in the plane of the ring) | No: the centre lies in the empty space inside the ring |
| (iv) Cube | At the point of intersection of the body diagonals (centre of the cube) | Yes (inside) |
- The geometric centre of each of these symmetrical bodies is the CM, because the distribution of mass is symmetric about it.
- Does the CM necessarily lie inside the body? No. It lies within the body for solid bodies of regular shape, but not for bodies of special shapes: a ring or circular hoop (CM at the centre, in the hole), a hollow sphere or hollow cylinder (CM at the centre of the hollow), a horse-shoe (U-shaped) magnet, a boomerang, a bent rod or an L-shaped bracket may have the CM outside the material.
- The CM is a mathematical point characterising the distribution of mass; it behaves as if all the mass were concentrated there (Section 6.3).
Examples of a CM outside the body. A ring; a hollow pipe; a bangle; a crescent; a banana (a curved body: the CM lies in the air on the concave side). The high-jumper’s ‘Fosbury flop’ technique makes use of this fact: by arching the body over the bar the CM can pass under the bar even though the body goes over it.
Extra depth. The CM of a symmetric body of non-uniform density, such as a cricket ball with a heavier side, is not at the geometric centre. For a body in a uniform gravitational field the CM coincides with the centre of gravity (CG): the point where the body can be balanced. A ring can be balanced on a finger only at points on its circumference: its CM/CG at the centre in space cannot be supported directly. The centre of mass of a system of two particles lies on the line joining them, nearer to the heavier one (Fig. 6.6).
Conclusion: (i) centre; (ii) mid-point of the axis; (iii) centre of the ring; (iv) intersection of the diagonals. No: e.g. a ring or hollow sphere has its CM outside the material.
Ex 6.2 — In the HCl molecule, the separation between the nuclei of the two atoms is about 1.27 Å (1 Å = 10−10 m). Find the approximate location of the CM of the molecule, given that a chlorine atom is about 35.5 times as massive as a hydrogen atom and nearly all the mass of an atom is concentrated in its nucleus.
Concept. Treat the molecule as two point masses at the nuclei, a hydrogen atom of mass m and a chlorine atom of mass 35.5 m, separated by 1.27 Å. The CM of two particles lies on the line joining them at a position determined by X = (m1x1 + m2x2)/(m1 + m2). Choose the origin conveniently at the chlorine nucleus.
- Let the origin be at the chlorine nucleus: xCl = 0 (mass 35.5 m); xH = 1.27 Å (mass m).
- X = (35.5 m × 0 + m × 1.27)/(35.5 m + m) = 1.27/36.5 Å = 0.035 Å.
- Hence the CM is located on the line joining the two nuclei at about 0.035 Å (3.5 × 10−12 m) from the chlorine nucleus, i.e. 1.235 Å from the hydrogen nucleus (the CM is very close to the Cl nucleus, towards the H atom).
| Quantity | Value |
|---|---|
| Separation of nuclei | 1.27 Å |
| Mass ratio mCl : mH | 35.5 : 1 |
| Distance of CM from Cl | 1.27/36.5 = 0.035 Å |
| Distance of CM from H | 1.27 − 0.035 = 1.235 Å |
| Ratio of distances (Cl : H) | 1 : 35.5 (inverse of the mass ratio) |
Rule: the CM divides the line joining the two masses in the inverse ratio of the masses: xCl : xH = mH : mCl = 1 : 35.5. The lighter atom is therefore much farther from the CM.
Extra depth. This explains why in the HCl molecule it is essentially the hydrogen atom that moves when the molecule vibrates or rotates: the heavy chlorine atom stays almost at the CM. This idea is important in molecular spectroscopy: the effective mass (reduced mass) of the HCl molecule is nearly equal to the mass of the hydrogen atom: μ = m1m2/(m1 + m2) = 35.5m/36.5 = 0.97 m. The moment of inertia of the molecule about the CM is I = m1x12 + m2x22 = μr2 = 0.97 × (1.67 × 10−27 kg) × (1.27 × 10−10)2 = 2.6 × 10−47 kg m2.
Conclusion: The CM of the HCl molecule is on the line joining the nuclei, about 0.035 Å from the chlorine nucleus (towards hydrogen).
Ex 6.3 — A child sits stationary at one end of a long trolley moving uniformly with a speed V on a smooth horizontal floor. If the child gets up and runs about on the trolley in any manner, what is the speed of the CM of the (trolley + child) system?
Concept. The system trolley + child is acted upon by no external horizontal force (the floor is smooth: no friction) and the vertical forces (weights and normal reaction) cancel. The forces exerted by the child on the trolley (when running) and by the trolley on the child are internal forces (equal and opposite) and cannot change the motion of the CM of the system (M A = Fext = 0).
- External force on the system (horizontal) = 0.
- Therefore the acceleration of the CM is zero: A = Fext/M = 0.
- So the velocity of the CM remains constant: it was V initially (the trolley and child moved together at V), hence it remains V however the child runs about on the trolley.
| Quantity | Before | After the child runs about |
|---|---|---|
| Total momentum P = MVcm | (M + m)V | (M + m)V (unchanged) |
| Speed of the CM | V | V |
| Speed of the trolley alone | V | changes (the trolley speeds up/slows down as the child moves) |
| Speed of the child alone | V (with the trolley) | changes (relative to the floor) |
Detail. If the child runs forward (relative to the trolley) the trolley slows down (momentum of the trolley decreases because the child pushes it backward), and when the child stops running the original common velocity V is restored (total momentum conserved): (M + m)V = MVT + mVC, with VT and VC changing but the weighted average staying V.
Extra depth. This example shows the power of the CM concept: the complicated motions of the parts do not change the CM motion in the absence of an external force. The same is true for a person walking on a raft in still water (the CM of person + raft stays fixed in the horizontal direction): if he walks to the right the raft moves to the left. Fireworks exploding in the air, a rocket in free space, and a boat crew all obey the same rule: the CM follows the path determined by the external forces only.
Conclusion: The speed of the CM of the (trolley + child) system remains V.
Ex 6.4 — Show that the area of the triangle contained between the vectors a and b is one half of the magnitude of a × b.
Concept. The vector (cross) product has magnitude |a × b| = ab sinθ, where θ is the angle between a and b. If the two vectors are drawn from a common point O as two sides of a triangle, we can compare the area with ab sinθ.
- Draw the vectors a = OP and b = OQ from O with angle θ between them; join P and Q to form triangle OPQ.
- Take OP (length a) as the base. Drop a perpendicular from Q to the line OP: its length is the height h = OQ sinθ = b sinθ.
- Area of triangle OPQ = ½ × base × height = ½ × a × b sinθ = ½ ab sinθ.
- But |a × b| = ab sinθ. Therefore area of triangle = ½|a × b|. Proved.
| Quantity | Expression |
|---|---|
| Magnitude of a × b | ab sinθ |
| Area of the parallelogram on a and b | base × height = a × b sinθ = |a × b| |
| Area of the triangle OPQ | ½ |a × b| |
Example. For a = 3î and b = 4ĵ (perpendicular): a × b = 12k̂, |a × b| = 12, so the area of the triangle is 6 (the right triangle with legs 3 and 4: ½ × 3 × 4 = 6 ✓).
Extra depth. The magnitude of the vector product is the area of the parallelogram whose adjacent sides are the two vectors; the triangle is half of it (the diagonal divides the parallelogram into two equal triangles). This geometric meaning is used in Kepler’s second law: the area swept per unit time by the radius vector, dA/dt = ½|r × v| = L/2m, is constant when the angular momentum is conserved. Using the determinant form, the area of a triangle with vertices at the origin, a and b in a plane is ½|axby − aybx|.
Conclusion: Area of the triangle = ½ a b sinθ = ½|a × b|.
Ex 6.5 — Show that a · (b × c) is equal in magnitude to the volume of the parallelepiped formed on the three vectors a, b and c.
Concept. Let the three vectors a, b and c be drawn from a common point O and form the three adjacent edges of a parallelepiped. The volume of a parallelepiped is (area of the base) × (height). Take the parallelogram formed by b and c as the base; its area is |b × c| and the vector b × c is perpendicular to the base.
- The base is the parallelogram on b and c: area of base = |b × c| = bc sinφ (φ = angle between b and c).
- The vector b × c = |b × c| n̂, where n̂ is the unit normal to the base. The height h of the parallelepiped is the perpendicular distance of the top face from the base, i.e. the component of a along n̂: h = a cosθ where θ is the angle between a and n̂ (the direction of b × c).
- Volume V = (area of base) × (height) = |b × c| × a cosθ.
- But the scalar product a · (b × c) = |a| |b × c| cosθ = a |b × c| cosθ, which equals V.
- Hence |a · (b × c)| = volume of the parallelepiped. (The triple product is positive if a, b, c form a right-handed system and negative otherwise; the volume is its magnitude.)
| Quantity | Meaning |
|---|---|
| b × c | vector normal to the base, magnitude = area of the base |
| a · (b × c) | (area of base) × (height) = volume (with sign for orientation) |
| Cyclic property | a · (b × c) = b · (c × a) = c · (a × b) |
| Determinant form | a · (b × c) = | ax ay az; bx by bz; cx cy cz | |
Example. For a = î, b = ĵ, c = k̂ (edges of a unit cube): b × c = î, a · (b × c) = î·î = 1 = volume of the unit cube.
Extra depth. If the triple product is zero, the three vectors are coplanar (the parallelepiped is flat, volume zero). The cyclic symmetry a · (b × c) = b · (c × a) = c · (a × b) follows because the volume does not depend on which face is taken as the base. The scalar triple product is used in physics for the volume of the unit cell of a crystal (a · (b × c) of the lattice vectors) and for the power of a torque.
Conclusion: a · (b × c) = |b × c|(a cosθ) = (area of the base) × (height) = volume of the parallelepiped.
Ex 6.6 — Find the components along the x, y, z axes of the angular momentum l of a particle, whose position vector is r with components x, y, z and momentum is p with components px, py and pz. Show that if the particle moves only in the x-y plane the angular momentum has only a z-component.
Concept. The angular momentum of a particle about the origin is l = r × p. Write r = xî + yĵ + zk̂ and p = pxî + pyĵ + pzk̂ and expand the cross product using î × ĵ = k̂, ĵ × k̂ = î, k̂ × î = ĵ (and the reverse products with a minus sign; like unit vectors give zero).
- l = r × p = | î ĵ k̂ ; x y z ; px py pz |.
- Expanding the determinant: l = (y pz − z py)î + (z px − x pz)ĵ + (x py − y px)k̂.
- Hence the components are: lx = y pz − z py, ly = z px − x pz, lz = x py − y px.
- Motion in the x–y plane: z = 0 and pz = 0 (no component of position or momentum along z). Then lx = y(0) − 0 × py = 0; ly = 0 × px − x(0) = 0; and only lz = x py − y px survives.
- So for a particle moving in the x–y plane l = (x py − y px)k̂, i.e. the angular momentum is directed along the z-axis, perpendicular to the plane of motion (as the right-hand rule requires for r × p, since both r and p lie in the x–y plane).
| Component | Expression | Value for motion in the x–y plane (z = pz = 0) |
|---|---|---|
| lx | y pz − z py | 0 |
| ly | z px − x pz | 0 |
| lz | x py − y px | x py − y px (non-zero) |
Example. A particle at r = (3, 4, 0) m with p = (2, −1, 0) kg m s−1: lz = 3(−1) − 4(2) = −11 kg m2 s−1, lx = ly = 0: the angular momentum is 11 units along the −z axis (clockwise motion seen from +z).
Extra depth. In polar form lz = r p sinθ, which equals mvr for circular motion (θ = 90°). In three dimensions the three components are the same as the 3 independent torque/angular momentum components used in the study of rotation; l is perpendicular to both r and p, so l · r = 0 and l · p = 0 (you can check: x lx + y ly + z lz = 0). A plane motion about a point in the plane has only one non-zero component, which is why in this chapter angular momentum for planar problems is treated as a scalar with a sign.
More to know — angular momentum of a particle in circular motion. For uniform circular motion in the x–y plane with radius r and angular speed ω: x = r cosωt, y = r sinωt, px = −mrω sinωt, py = mrω cosωt, so lz = xpy − ypx = mr2ω(cos2 + sin2) = mr2ω = mvr, constant in time and along +z for counter-clockwise motion. The same formula gives L = Iω for a rigid body. The angular momentum of a particle moving in a straight line with constant velocity is also constant (Example 6.6) and equals mv times the perpendicular distance of the line from the origin.
Conclusion: lx = ypz − zpy, ly = zpx − xpz, lz = xpy − ypx; for planar motion in the xy-plane only lz is non-zero.
Ex 6.7 — Two particles, each of mass m and speed v, travel in opposite directions along parallel lines separated by a distance d. Show that the angular momentum vector of the two particle system is the same whatever be the point about which the angular momentum is taken.
Concept. The angular momentum of the system about a point O is L = r1 × p1 + r2 × p2, where r1, r2 are the position vectors of the two particles from O and p1 = mv, p2 = −mv are their momenta (equal in magnitude, opposite in direction). We show that L does not depend on the position of O.
- Let the particles be at positions r1 and r2 relative to an arbitrary origin O. The velocities are v and −v, so p1 = mv and p2 = −mv.
- L = r1 × mv + r2 × (−mv) = m(r1 − r2) × v.
- The vector r1 − r2 = r12 is the position vector of particle 1 relative to particle 2: it depends only on the positions of the two particles, not on the origin (any shift of the origin by a vector a changes r1 and r2 by the same a and leaves the difference unchanged).
- Therefore L = m r12 × v is independent of the choice of O. Its magnitude is m v (r12 sinθ) = m v d, because the component of r12 perpendicular to the (parallel) lines of motion is the separation d; its direction is perpendicular to the plane containing the two lines of motion.
| Origin chosen | L (magnitude) | Direction |
|---|---|---|
| O on the line of particle 1 | m v d | perpendicular to the plane of motion (right-hand rule) |
| O midway between the lines | m v (d/2) + m v (d/2) = m v d | same |
| O outside the two lines | m v (x + d) − m v x = m v d | same |
Check with distances. If O lies between the two lines at perpendicular distances x_1 and x_2 from them (x_1 + x_2 = d), the two contributions have the same sense and add up: mvx_1 + mvx_2 = mvd. If O lies outside, at distances x and x + d from the lines, the contributions have opposite senses: mv(x + d) − mvx = mvd. The result is always mvd.
Extra depth. The result is a special case of a general theorem: the angular momentum of a system depends on the choice of the origin by an amount R × P where R is the shift and P the total momentum. Here the total momentum is p1 + p2 = 0, so the angular momentum is independent of the origin. The two particles form a ‘couple’-like arrangement (equal and opposite momenta along different lines), whose angular momentum, like the moment of a couple of forces (Example 6.7), is independent of the reference point.
Conclusion: The total angular momentum L = m (r1 − r2) × v = mvd (perpendicular to the plane) is the same about every point.
Ex 6.8 — A non-uniform bar of weight W is suspended at rest by two strings of negligible weight as shown in Fig. 6.33. The angles made by the strings with the vertical are 36.9° and 53.1° respectively. The bar is 2 m long. Calculate the distance d of the centre of gravity of the bar from its left end.
Concept. The bar is in equilibrium under three forces: its weight W (acting at the CG, a distance d from the left end), and the tensions T1 (left string, 36.9° to the vertical) and T2 (right string, 53.1° to the vertical). Equilibrium requires (i) ΣFx = 0, (ii) ΣFy = 0 (translational) and (iii) Στ = 0 (rotational), i.e. torques about any point sum to zero.
- Use sin36.9° = 0.6, cos36.9° = 0.8, sin53.1° = 0.8, cos53.1° = 0.6.
- Horizontal: T1 sin36.9° = T2 sin53.1° ⇒ 0.6 T1 = 0.8 T2 ⇒ T1 = (4/3)T2.
- Vertical: T1 cos36.9° + T2 cos53.1° = W ⇒ 0.8 T1 + 0.6 T2 = W ⇒ 0.8(4/3)T2 + 0.6T2 = W ⇒ (16/15 + 9/15) T2 = (5/3) T2 = W ⇒ T2 = 0.6 W and T1 = 0.8 W.
- Torques about the left end (taking anticlockwise positive): the weight acts downward at distance d (clockwise torque W d); the right string’s vertical component T2 cos53.1° acts upward at distance 2 m (anticlockwise torque T2 cos53.1° × 2); the left tension passes through the left end (zero torque) and its horizontal components act along the line of the bar (no torque about the end).
- Rotational equilibrium: T2 cos53.1° × 2 = W d ⇒ 0.6W × 0.6 × 2 = W d ⇒ d = 0.72 m.
| Quantity | Value |
|---|---|
| T1 | 0.8 W |
| T2 | 0.6 W |
| Torque of T2 about the left end | 0.6W × 0.6 × 2 m = 0.72 W m |
| Distance d | 0.72 m from the left end |
Check (torques about the right end): W (2 − d) = T1 cos36.9° × 2 ⇒ W(2 − d) = 0.8W × 0.8 × 2 = 1.28W ⇒ 2 − d = 1.28 ⇒ d = 0.72 m ✓.
Extra depth. The CG is closer to the left end (0.72 m from the left, 1.28 m from the right), as expected from the fact that the left string, nearer to the vertical, carries the larger tension (0.8W): the larger share of the weight is supported near the CG’s side. A uniform bar would have its CG at d = 1 m (the middle). The method — resolve forces, then take moments about a convenient point where unknown forces pass — is the standard approach to rigid-body equilibrium problems.
Conclusion: d = 0.72 m from the left end.
Ex 6.9 — A car weighs 1800 kg. The distance between its front and back axles is 1.8 m. Its centre of gravity is 1.05 m behind the front axle. Determine the force exerted by the level ground on each front wheel and each back wheel.
Concept. The car is in equilibrium on level ground: the total upward reaction of the ground equals the weight, and the torques about any point vanish. Let Rf be the total reaction on the two front wheels and Rb on the two back wheels. The weight acts at the CG, 1.05 m behind the front axle, i.e. 1.8 − 1.05 = 0.75 m in front of the back axle.
- Weight W = 1800 kg × 9.8 m s−2 = 17640 N (taking g = 9.8 m s−2; 1800 kg wt).
- Translational equilibrium: Rf + Rb = W = 17640 N.
- Rotational equilibrium (torques about the back axle): Rf × 1.8 = W × 0.75 ⇒ Rf = 17640 × 0.75/1.8 = 7350 N.
- Rb = 17640 − 7350 = 10290 N.
- The force on each wheel: front wheel = Rf/2 = 3675 N (≈ 375 kg wt); back wheel = Rb/2 = 5145 N (≈ 525 kg wt).
| Quantity | Axle total | Per wheel |
|---|---|---|
| Front | 7350 N (750 kg wt) | 3675 N |
| Back | 10290 N (1050 kg wt) | 5145 N |
| Total | 17640 N (1800 kg wt) |
Check by torques about the front axle: Rb × 1.8 = W × 1.05 ⇒ Rb = 17640 × 1.05/1.8 = 10290 N ✓.
Extra depth. The back wheels carry more weight (58%) because the CG is nearer to the back axle (0.75 m) than to the front (1.05 m). The load on the wheels is inversely proportional to the distance of the CG from the respective axle: Rf : Rb = 0.75 : 1.05 = 5 : 7. This is why heavy loads are put towards the rear in a truck, and why braking transfers weight to the front wheels (dynamic load transfer). In the exercise the ‘1800 kg’ is a mass and the forces are weights in newtons (using g = 9.8 m s−2).
Conclusion: Front wheel: 3675 N; back wheel: 5145 N (g = 9.8 m s−2).
Ex 6.10 — Torques of equal magnitude are applied to a hollow cylinder and a solid sphere, both having the same mass and radius. The cylinder is free to rotate about its standard axis of symmetry, and the sphere is free to rotate about an axis passing through its centre. Which of the two will acquire a greater angular speed after a given time.
Concept. Rotational dynamics: τ = Iα, so the angular acceleration α = τ/I. Starting from rest, the angular speed after time t is ω = αt = τt/I. For the same torque and time, the body with the smaller moment of inertia attains the greater angular speed. Compare the moments of inertia from Table 6.1.
| Body | Axis | Moment of inertia | Angular acceleration α = τ/I |
|---|---|---|---|
| Hollow cylinder (mass M, radius R) | its axis | I1 = MR2 | τ/MR2 |
| Solid sphere (mass M, radius R) | through its centre (diameter) | I2 = (2/5)MR2 | 5τ/2MR2 |
- I1 = MR2 and I2 = (2/5)MR2 = 0.4 MR2; so I2 < I1.
- α1 = τ/I1 and α2 = τ/I2 ⇒ α2/α1 = I1/I2 = 5/2 = 2.5.
- After time t (starting from rest) ω = αt, so ωsphere/ωcylinder = 2.5.
- Therefore the solid sphere acquires the greater angular speed (2.5 times that of the hollow cylinder).
Physical reason. In the hollow cylinder all the mass is at the maximum distance R from the axis, which gives the largest possible I for the given M and R (I = MR2). In the solid sphere much of the mass is near the axis, so I is small, and the same torque produces a large angular acceleration.
Extra depth. The moment of inertia plays the role of mass in rotation: the larger the I, the harder to start or stop the rotation. This is why a flywheel (a large-I wheel with mass concentrated at the rim) smooths out engine fluctuations, while a figure skater reduces I by pulling the arms close to the body in order to spin fast. The result ω ∝ 1/I also explains why a hollow pipe is harder to spin than a solid rod of the same mass and radius.
More to know — moments of inertia compared. For the same mass M and radius R: hollow cylinder (or ring about its axis) MR2; solid cylinder MR2/2; hollow sphere 2MR2/3; solid sphere 2MR2/5. A larger I means a smaller angular acceleration for the same torque and also a smaller kinetic energy for the same angular momentum (K = L2/2I). When bodies roll down an incline the one with the smallest I/MR2 arrives first: solid sphere (0.4) beats solid cylinder (0.5), which beats hollow sphere (0.67), which beats hollow cylinder or ring (1) — a standard NEET question related to this exercise.
Conclusion: The solid sphere acquires the greater angular speed (2.5 times that of the hollow cylinder) since its moment of inertia is smaller.
Ex 6.11 — A solid cylinder of mass 20 kg rotates about its axis with angular speed 100 rad s−1. The radius of the cylinder is 0.25 m. What is the kinetic energy associated with the rotation of the cylinder? What is the magnitude of angular momentum of the cylinder about its axis?
Concept. For rotation about a fixed axis the kinetic energy is K = ½Iω2 and the angular momentum is L = Iω. For a solid cylinder about its own axis the moment of inertia is I = ½MR2 (Table 6.1).
- Mass M = 20 kg, radius R = 0.25 m, ω = 100 rad s−1.
- Moment of inertia I = ½MR2 = ½ × 20 × (0.25)2 = 10 × 0.0625 = 0.625 kg m2.
- Kinetic energy of rotation K = ½Iω2 = ½ × 0.625 × (100)2 = ½ × 0.625 × 104 = 3125 J (≈ 3.1 × 103 J).
- Angular momentum L = Iω = 0.625 × 100 = 62.5 J s (kg m2 s−1).
| Quantity | Formula | Value |
|---|---|---|
| Moment of inertia | ½MR2 | 0.625 kg m2 |
| Rotational kinetic energy | ½Iω2 | 3125 J |
| Angular momentum | Iω | 62.5 kg m2 s−1 |
| Check: K = Lω/2 | 62.5 × 100/2 | 3125 J ✓ |
Relations: K = L2/(2I) = (62.5)2/(2 × 0.625) = 3125 J. The linear speed of a point on the rim is v = ωR = 100 × 0.25 = 25 m s−1 (90 km h−1), and a particle on the rim has a centripetal acceleration ω2R = 2500 m s−2.
Extra depth. The energy stored in the spinning cylinder (3.1 kJ) is large relative to its size: this is how flywheels store energy (used in some buses and in energy-storage devices). If the cylinder had been hollow (I = MR2 = 1.25 kg m2), at the same ω the energy would be 6250 J and L = 125 J s: twice as much, because the mass is concentrated at the rim.
More to know — rotational analogues. Every translational formula has a rotational partner: K = ½Mv2 ↔ ½Iω2; p = Mv ↔ L = Iω; F = Ma ↔ τ = Iα; P = Fv ↔ τω. For the cylinder of the exercise, stopping it in 10 s needs a constant retarding torque τ = Iω/t = 0.625 × 100/10 = 6.25 N m, and the work done in stopping it equals its kinetic energy, 3125 J, which would appear as heat in the brake. Energy stored in a flywheel is proportional to Iω2, so doubling the speed stores four times as much energy.
Conclusion: K = 3125 J (3.1 × 103 J) and L = 62.5 kg m2 s−1.
Ex 6.12 — (a) A child stands at the centre of a turntable with his two arms outstretched. The turntable is set rotating with an angular speed of 40 rev/min. How much is the angular speed of the child if he folds his hands back and thereby reduces his moment of inertia to 2/5 times the initial value? Assume that the turntable rotates without friction. (b) Show that the child’s new kinetic energy of rotation is more than the initial kinetic energy of rotation. How do you account for this increase in kinetic energy?
Concept. With no external torque (frictionless turntable) the angular momentum of the child + turntable is conserved: I1ω1 = I2ω2. The child changes his moment of inertia by moving his arms, which changes the angular speed inversely. The kinetic energy K = ½Iω2 is not conserved: it changes because of internal work done by the child.
(a) New angular speed
- I1 = I (initial), ω1 = 40 rev/min; I2 = (2/5)I.
- Conservation of angular momentum: I1ω1 = I2ω2 ⇒ ω2 = (I1/I2)ω1 = (5/2) × 40 = 100 rev/min.
- In rad s−1: ω1 = 2π × 40/60 = 4.19 rad s−1; ω2 = 10.5 rad s−1.
(b) Rotational kinetic energy
- K1 = ½I1ω12, K2 = ½I2ω22.
- K2/K1 = (I2/I1)(ω2/ω1)2 = (2/5)(5/2)2 = (2/5)(25/4) = 5/2 = 2.5.
- So the new kinetic energy is 2.5 times the initial one: it has increased (by 150%).
- Source of the extra energy: the child does work against the ‘outward’ (centrifugal-like) tendency of the arms while pulling them in: the muscular (internal) force acting along the displacement of the arms does positive work, converting the child’s chemical (internal) energy into rotational kinetic energy. The total energy is conserved when the child’s chemical energy is counted.
| Quantity | Initial | Final | Ratio |
|---|---|---|---|
| Moment of inertia | I | 2I/5 | 0.4 |
| Angular speed | 40 rev/min | 100 rev/min | 2.5 |
| Angular momentum Iω | I × 40 | (2I/5) × 100 = I × 40 | 1 (conserved) |
| Kinetic energy ½Iω2 | K | 2.5K | 2.5 |
General relation: K = L2/(2I); at constant L, K ∝ 1/I. Reducing I to 2/5 increases K by 5/2. The ‘work done by the child’ is 1.5 K1.
Extra depth. The same physics governs a skater who spins faster when pulling the arms in, a diver in a tuck, the collapse of a star (a rotating cloud of gas contracting spins faster: neutron stars may rotate hundreds of times per second) and an ice dancer. Angular momentum is conserved because the net external torque is zero (the turntable is frictionless and the child’s weight is balanced by the normal reaction along the axis). A paradox only arises if one forgets that the internal forces (muscles) can do work even though they exert no net external torque.
Conclusion: (a) 100 rev/min; (b) K2/K1 = 2.5: the increase comes from the work done by the child (internal energy).
Ex 6.13 — A rope of negligible mass is wound round a hollow cylinder of mass 3 kg and radius 40 cm. What is the angular acceleration of the cylinder if the rope is pulled with a force of 30 N? What is the linear acceleration of the rope? Assume that there is no slipping.
Concept. The tension (pull) of the rope applies a torque about the axis of the cylinder: τ = F R. The rotational equation of motion τ = Iα then gives the angular acceleration, with I = MR2 for a hollow cylinder about its axis. If the rope does not slip on the cylinder, the linear acceleration of the rope equals the tangential acceleration of the rim: a = αR.
- M = 3 kg, R = 40 cm = 0.40 m, F = 30 N.
- Torque τ = F R = 30 × 0.40 = 12 N m.
- Moment of inertia of the hollow cylinder (thin-walled) about its axis I = MR2 = 3 × (0.40)2 = 0.48 kg m2.
- Angular acceleration α = τ/I = 12/0.48 = 25 rad s−2.
- Linear acceleration of the rope a = αR = 25 × 0.40 = 10 m s−2 (equal to the tangential acceleration of the rim).
| Quantity | Value |
|---|---|
| Torque | 12 N m |
| I = MR2 | 0.48 kg m2 |
| α | 25 rad s−2 |
| a = αR | 10 m s−2 |
Check by linear dynamics? For a hollow cylinder pulled by a rope with force F, the rope acceleration a = F R2/I = F/M = 30/3 = 10 m s−2: the same as for a free particle of mass M pulled by F, because for a thin-walled cylinder all the mass is at the rim, so the rotational inertia equals the translational inertia M when expressed in rim terms.
Extra depth. For a solid cylinder (I = ½MR2) the same pull would give α = 50 rad s−2 and a = 20 m s−2, twice as large, since its moment of inertia is half. If the cylinder were free to move as well (not fixed on an axis), the equations would change (translation + rotation). Here the cylinder is on a fixed axis, and the force and the rope are assumed ideal: the hand supplies a constant 30 N.
More to know — solid versus hollow cylinder. The acceleration of a rope wound on a cylinder fixed on an axis is a = F R2/I. With I = MR2 (hollow) a = F/M = 10 m s−2; with I = ½MR2 (solid) a = 2F/M = 20 m s−2. If the cylinder is free to roll down while the rope end is fixed (a yo-yo), the acceleration of the centre is a = g/(1 + I/MR2): g/2 for a hollow cylinder and 2g/3 for a solid cylinder. These comparisons show how a larger moment of inertia gives a smaller angular acceleration.
Conclusion: α = 25 rad s−2; linear acceleration of the rope = 10 m s−2.
Ex 6.14 — To maintain a rotor at a uniform angular speed of 200 rad s−1, an engine needs to transmit a torque of 180 N m. What is the power required by the engine? (Note: uniform angular velocity in the absence of friction implies zero torque. In practice, applied torque is needed to counter frictional torque). Assume that the engine is 100% efficient.
Concept. The power transmitted by a torque τ to a body rotating with angular velocity ω is P = τω (the rotational analogue of P = Fv). At uniform angular speed the engine’s torque only balances the frictional torque (net torque zero, so no angular acceleration), but it continuously supplies energy at the rate τω to compensate for the heat produced by friction.
- Torque τ = 180 N m, angular speed ω = 200 rad s−1.
- Power P = τω = 180 × 200 = 36000 W = 3.6 × 104 W (36 kW).
- Since the engine is assumed 100% efficient, this is also the power input; in horse power: 36000/746 = 48 hp.
| Quantity | Value |
|---|---|
| Torque τ | 180 N m |
| Angular speed ω | 200 rad s−1 (= 1910 rev/min) |
| Power τω | 3.6 × 104 W = 36 kW ≈ 48 hp |
Energy in one minute: E = Pt = 36 kW × 60 s = 2.16 MJ = 0.6 kWh; all of it appears as heat generated by friction in the bearings, since the kinetic energy of the rotor does not change at constant ω.
Extra depth. Derivation: dW = τdθ, so P = dW/dt = τdθ/dt = τω. The torque times the rotation speed is also the way vehicle power is specified: engine power (kW) = torque (N m) × 2π × (rev/min)/60000. For 1910 rev/min and 180 N m this reproduces 36 kW. At the same power a lower speed demands a higher torque, which is why gears are used.
More to know — engines and torque. Engine power P = τω, so for a fixed power the torque is inversely proportional to the speed: the same 36 kW engine delivers 180 N m at 200 rad s−1 but 360 N m at 100 rad s−1. Gearboxes convert high speed/low torque into low speed/high torque for climbing a hill. In an electric motor the torque is proportional to the current. The unit of torque (N m) is dimensionally the joule but torque is a vector while energy is a scalar; do not call torque ‘joule’.
Conclusion: The power required is 3.6 × 104 W (36 kW).
Ex 6.15 — From a uniform disk of radius R, a circular hole of radius R/2 is cut out. The centre of the hole is at R/2 from the centre of the original disc. Locate the centre of gravity of the resulting flat body.
Concept. Use the superposition (negative mass) method: the original full disc = (the remaining body) + (the hole piece). The CM of the whole disc is at its centre O; the CM of the cut-out disc is at its own centre, at a distance R/2 from O. Treat the remaining body as the whole disc minus the hole. The CG coincides with the CM for a flat body in uniform gravity.
- Let the mass per unit area be σ. Mass of the full disc M = σπR2. Mass of the removed disc (radius R/2) = σπ(R/2)2 = M/4. Mass of the remaining body = M − M/4 = 3M/4.
- Take the origin at the centre O of the original disc and the x-axis along the line from O to the centre of the hole (hole centre at x = +R/2).
- CM of the full disc (at O) = [ (3M/4) xrem + (M/4)(R/2) ]/M = 0 (since the full disc is symmetric about O).
- So (3M/4) xrem + MR/8 = 0 ⇒ xrem = −(MR/8)/(3M/4) = −R/6.
- Hence the CG of the remaining body is at a distance R/6 from the centre O of the original disc, on the side opposite to the hole (on the line joining O to the centre of the hole).
| Part | Mass | CM position (from O) |
|---|---|---|
| Full disc | M | 0 |
| Hole (removed) | M/4 | +R/2 |
| Remaining body | 3M/4 | −R/6 |
Check by direct moments: M(0) = (3M/4)(−R/6) + (M/4)(R/2) = −MR/8 + MR/8 = 0 ✓.
Extra depth. The method of treating a hole as a body of negative mass is a standard trick for finding the CM of bodies with cut-outs. It applies equally to moments of inertia and to gravitational and electrostatic fields. The remainder balances at a point on the side away from the hole, which makes sense: removing mass from the right side shifts the CM to the left. In the general case with a hole of radius r whose centre is at distance a from O, the shift is x = −(r2 a)/(R2 − r2).
Conclusion: The CG of the remaining body is at R/6 from the centre of the original disc, on the side opposite to the hole.
Ex 6.16 — A metre stick is balanced on a knife edge at its centre. When two coins, each of mass 5 g are put one on top of the other at the 12.0 cm mark, the stick is found to be balanced at 45.0 cm. What is the mass of the metre stick?
Concept. A uniform metre stick has its centre of gravity at the 50.0 cm mark: this is where it balances on its own. With the two coins on the 12.0 cm mark, the system balances at 45.0 cm, so the total torque of the weights about the 45.0 cm mark must vanish (principle of moments: clockwise moment = anticlockwise moment).
- Mass of the coins mc = 2 × 5 g = 10 g at x = 12.0 cm; let the mass of the stick be M at x = 50.0 cm (its CG).
- Pivot (knife edge) at x = 45.0 cm. Distance of the coins from the pivot = 45.0 − 12.0 = 33.0 cm (left of the pivot); distance of the stick’s CG from the pivot = 50.0 − 45.0 = 5.0 cm (right of the pivot).
- Moments about the pivot: 10 g × 33.0 cm = M × 5.0 cm (g cancels).
- M = 10 × 33.0/5.0 = 66 g.
| Item | Mass | Position | Distance from pivot (45 cm) |
|---|---|---|---|
| Two coins | 10 g | 12.0 cm | 33.0 cm (left) |
| Metre stick | M | 50.0 cm (CG) | 5.0 cm (right) |
| Balance condition | 10 × 33 = M × 5 | M = 66 g |
Check using the CM: CM of the system = (10 × 12 + 66 × 50)/(10 + 66) = (120 + 3300)/76 = 3420/76 = 45.0 cm ✓, which is the observed balance point.
Extra depth. This is a practical method to find the mass of an object using a balance of known masses (the principle of moments), the basis of the beam balance, the lever and the steelyard. In the experimental physics of metre bridge or metre-stick balances the knife edge is moved until the stick is balanced; the position gives the CM of the combined system. Note that the mass of the stick, 66 g, is realistic for a wooden metre stick.
More to know — the principle of moments in practice. A balance works by equating moments: m1d1 = m2d2. A beam balance compares masses; a steelyard uses a sliding known mass; the metre-stick method used here is an inexpensive way to weigh light objects: with the pivot at 45 cm and a 10 g load at 12 cm one finds a stick mass of 66 g. Sensitivity: moving the coins to the 6 cm mark would shift the balance point to (10 × 6 + 66 × 50)/76 = 44.2 cm; the shift of 0.8 cm is easily measurable, so a few grams can be weighed to within a gram.
Conclusion: The mass of the metre stick is 66 g.
Ex 6.17 — The oxygen molecule has a mass of 5.30 × 10−26 kg and a moment of inertia of 1.94 × 10−46 kg m2 about an axis through its centre perpendicular to the lines joining the two atoms. Suppose the mean speed of such a molecule in a gas is 500 m/s and that its kinetic energy of rotation is two thirds of its kinetic energy of translation. Find the average angular velocity of the molecule.
Concept. A diatomic molecule has translational kinetic energy Kt = ½mv2 and rotational kinetic energy Kr = ½Iω2 about the perpendicular axis through its centre. The data give Kr = (2/3)Kt, from which ω is found.
- m = 5.30 × 10−26 kg, v = 500 m s−1, I = 1.94 × 10−46 kg m2.
- Kt = ½mv2 = ½ × 5.30 × 10−26 × (500)2 = ½ × 5.30 × 10−26 × 2.5 × 105 = 6.625 × 10−21 J.
- Kr = (2/3)Kt = (2/3) × 6.625 × 10−21 = 4.417 × 10−21 J.
- Kr = ½Iω2 ⇒ ω2 = 2Kr/I = 2 × 4.417 × 10−21/1.94 × 10−46 = 4.55 × 1025.
- ω = √(4.55 × 1025) = 6.75 × 1012 rad s−1.
| Quantity | Value |
|---|---|
| Translational KE | 6.6 × 10−21 J |
| Rotational KE (2/3 of it) | 4.4 × 10−21 J |
| ω2 = 2Kr/I | 4.55 × 1025 rad2 s−2 |
| ω | 6.75 × 1012 rad s−1 |
Comparison. The rotation frequency ν = ω/2π = 1.07 × 1012 Hz (about 1012 revolutions per second, in the far-infrared region). This is typical of molecular rotations. The angular momentum of the molecule L = Iω = 1.94 × 10−46 × 6.75 × 1012 = 1.31 × 10−33 J s, which is of the order of the Planck constant h/2π (1.05 × 10−34 J s): rotational motion at atomic level is quantised.
Extra depth. The factor 2/3 has been chosen to be consistent with the equipartition of energy in the kinetic theory of gases (Chapter 12): for a diatomic molecule at room temperature there are 3 translational and 2 rotational degrees of freedom, each with ½kT, so Kr/Kt = 2/3. This exercise therefore links mechanics to thermodynamics: the average angular velocity (6.75 × 1012 rad s−1) of an oxygen molecule at room temperature is enormous compared with everyday rotations.
Conclusion: The average angular velocity of the oxygen molecule is 6.75 × 1012 rad s−1.